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NanoBPM Update – Results Resolution Results Best resolution recorded so far was during April '06: Position:15.6nm Tilt:2.1rad From simulation work, electronic, thermal and vibrational noise not dominant. LCABD WP 4.2 Review, 24 th September Mark Slater ~60kHz ~0.25C ~8 hours Temperature Frequency changes over the course of 8 hours have been correlated with temperature changes of the BPMs The change seen is in reasonable agreement with that predicted from thermal expansion arguments Now published in NIM: A578:1-22,2007

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LCABD WP 4.2 Review, 24 th September Mark Slater ESA 2006 (T474) Update Final analysis of the data taken in 2006 is almost complete A lot has been learned from this data: Algorithm optimisation Calibration optimisation Dominant Systematics Required hardware upgrades

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ESA 2006 (T474) Results – Calibration Stability LCABD WP 4.2 Review, 24 th September Mark Slater Two types of calibration were used Corrector – enables calibration of all BPMs Mover – Accurate steps and can use outer BPMs to remove beam jitter More accurate calibrations could be found by using the mover calibration for one BPM to correct the those of the others Over a 20 hour period, the variation in calibration constants were found to be: Frequency: ~5kHz IQ Phase: 0.01 rad Scale: ~1% Given a typical offset of ~200 m, this was predicted to have the following effect Precision: ~150nm Accuracy: ~2-10μm Mover Cals Corrector Cals

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LCABD WP 4.2 Review, 24 th September Mark Slater ESA 2006 (T474) Results – Long Term Precision Stability The stability test was extended over a 20 hour period BPMs 1 and 2 were limited by the thermal stability of the electronics BPM 11 had a significant shift in frequency and a consequent change in calibration after 8 hours * Results from only 8 hours rather than 20 hours NOTE: All values in μm `Linked' refers to predicting the position at BPM 3 using BPMs 1-2 and 9-11 BPMs 3-5 BPMs 9-11

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ESA 2006 (T474) Results – Systematics LCABD WP 4.2 Review, 24 th September Mark Slater Several systematic sources were investigated Temperature Magnetic Field Vibrational Motion Charge Offset Temperature was found to be limiting the stability for most BPMs due to a change in calibration The Earth's field was found to produce an offset of 1.2 μm with a change in energy of 200 MeV Vibrational Motion was found to dominate the precision of BPM 4 There was some slight dependence of the residuals on position and charge Temperature Variation - ESA Temperature Variation – CHA Energy Variation vs. BPM Offset FFT of Vibrational Motion

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ESA 2006 (T474) – Conclusions The algorithms and systems used during 2006 running have been optimised to achieve the best precision and stability of the BPMs Precision of 250nm or better has been achieved and maintained for several BPMs over a minimum of 1 hour and a maximum of 8 hours Limitations on these results was found to be due to Electronic Noise Vibrational Motion Temperature Induced Calibration Changes All analysis for this paper has been completed using the `home- grown' libbpm library and has proved this code is ready for deployment in both online and offline systems A NIM paper is in its third (and hopefully final) draft Submission planned for end of September/beginning of October LCABD WP 4.2 Review, 24 th September Mark Slater

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ESA 2007 (T491) – Progress in 2007 A number of upgrades were carried out at ESA preceding this years running These included UK BPM, Mover and electronics Calibration Tone Calibration routine using Helmholtz Coils The major part of the upgrade was the installation of the four dipole magnets that formed a working spectrometer prototype Zygo InterferometerLocation of UK BPM LCABD WP 4.2 Review, 24 th September Mark Slater

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ESA 2007 (T491) – UK Hardware LCABD WP 4.2 Review, 24 th September Mark Slater An entire BPM system including mover and electronics has been designed and built by the group Installation of the electronics was performed in early 2007 with the BPM and mover installed in time for the July run The electronics were tested on BPMs already present (9-11) and comparable precisions were found as with the SLAC electronics (~150nm)‏ The mover and read back system was tested using the interferometer and was shown to work to a high degree of accuracy The BPM showed considerable cross-talk due to manufacturing problems A precision of 1.5 – 2 μm was achieved. See Bino's talk for more info on the UK equipment and future plans... Mover BPM Electronics

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The installed UK BPM electronics also included a CW calibration tone that could be used to check gain and phase variation The signal was split to go through the electronics of all the BPMs Using the 0.1 Hz trigger supplied by the SLAC control system, `online' calibration drifts could be corrected Initial (offline) checks have been made showing the variation of gain and phase with temperature ESA 2007 (T491) – Calibration Tone LCABD WP 4.2 Review, 24 th September Mark Slater (M. Christiakova/Berkeley)‏ Amplitude vs. Temperature Phase vs. Temperature

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ESA 2007 (T491) – Helmholtz Calibration Calibrating using the upstream steel correctors was found to be inaccurate due to drifts in the beam position during a cal step Another method was implemented that involved using helmholtz coils These could reach the desired field strength almost instantly and therefore a dithering calibration could be used Instead of averaging over events in each step, the scale was determined for a cal consisting of 5 events per step The scales were then averaged over several cals resulting in an improvement of scale variation from 40% to 5-10% ADC values were set indicating the position in the cal cycle allowing automation of the calibration LCABD WP 4.2 Review, 24 th September Mark Slater Position vs. Time ADC vs. Time

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LCABD WP 4.2 – Conclusions LCABD WP 4.2 Review, 24 th September Mark Slater The work completed in 2006 at both ATF and ESA has been written up and has either been or will be published. In summary, we have demonstrated: 15.6nm position resolution within a triplet ~800nm position resolution across a 40m beamline Stability within a triplet of a few hundred nm over 1-8 hours An understanding of the systematic issues dominating the BPMs In 2007, the following was achieved at ESA: Installation and commissioning of UK BPM, Mover and Electronics Improved calibration scheme Introduction of a calibration tone to improve on results from 2006 Installation and operation of a full spectrometer chicane Now on to LCABD2...